CMEs in the the Interplanetary Medium : analysis from the Sun to 1 AU

Details CMEs in the the Interplanetary Medium : analysis from the Sun to 1 AU CMEs in the the Interplanetary Medium : analysis from the Sun to 1 AU

Dec 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011agufmsh23a1946c&link_type=abstract

American Geophysical Union, Fall Meeting 2011, abstract #SH23A-1946

Astronomy and Astrophysics

Astrophysics

[7513] Solar Physics, Astrophysics, And Astronomy / Coronal Mass Ejections

Scientific paper

For many years, white light coronagraphs have provided information on the near Sun evolution of coronal mass ejections (CMEs). More recently, the Heliospheric Imager (HI) instruments aboard the STEREO mission are providing crucial remote sensing information on the interplanetary evolution of these events. Data from in situ instruments complete the overall characterization of interplanetary CMEs. In this work, we present an analysis of a CME from near the Sun to 1 AU using combined data from multiple spacecraft. We compare the propagation and evolution as observed in remote sensing data with in situ observations and derived parameters.

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